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<ri:Resource created="2010-10-28T21:07:46Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Spectroscopy of quasar binary candidates</title><shortName>J/ApJ/678/635</shortName><identifier>ivo://CDS.VizieR/J/ApJ/678/635</identifier><altIdentifier>doi:10.26093/cds/vizier.16780635</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Myers A.D.</name></creator><creator><name>Richards G.T.</name></creator><creator><name>Brunner R.J.</name></creator><creator><name>Schneider D.P.</name></creator><creator><name>Strand N.E.,Hall P.B.</name></creator><creator><name>Blomquist J.A.</name></creator><creator><name>York D.G.</name></creator><date role="Updated">2017-06-12T08:24:36Z</date><date role="Created">2010-10-28T21:07:46Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>spectroscopic-binary-stars</subject><subject>redshifted</subject><subject>quasars</subject><description>We present spectroscopy of binary quasar candidates, with component separations of 3"&lt;={Delta}{theta}&lt;6", selected from SDSS DR4 using kernel density estimation (KDE). Of our 27 new quasar pair observations, 10 are binary quasars, which doubles the number of known g&lt;21 binaries with 3"&lt;={Delta}{theta}&lt;6" separations. Several of our observed binaries are wide-separation lens candidates that merit additional higher resolution spectroscopy, as well as deep imaging to search for lensing galaxies. Our candidates are initially selected by UV excess (u-g&lt;1), but are otherwise selected irrespective of the relative colors of the quasar pair, and we thus use them to suggest optimal color similarity and photometric redshift approaches for targeting binary quasars or projected quasar pairs. We find that a third or more of all binary quasars have quite dissimilar components on the basis of a typical color similarity criterion ({chi}^2^_color_&lt;~20). From a sample that is complete on proper scales of 23.7h^-1^kpc&lt;R_prop_&lt;29.9h^-1^kpc, we determine the projected quasar correlation function.</description><source format="bibcode">2008ApJ...678..635M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/678/635</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/258">VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/496">J/AJ/135/496 : SDSS quasar lens search. II. 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